Moving away from the Near-Horizon Attractor of the Extreme Kerr Force-Free Magnetosphere
F. Camilloni, G. Grignani, T. Harmark, R. Oliveri, M. Orselli

TL;DR
This paper investigates force-free magnetospheres around extreme Kerr black holes, showing that deviations from the near-horizon attractor lead to magnetically-dominated solutions with finite angular momentum, using second-order perturbation analysis.
Contribution
It demonstrates how moving away from the NHEK attractor yields new magnetically-dominated solutions in extreme Kerr black holes.
Findings
Deviations from the NHEK attractor produce magnetically-dominated solutions.
Second-order perturbation analysis reveals finite angular momentum outflows.
Near-horizon attractor solutions are not unique when moving away from the NHEK limit.
Abstract
We consider force-free magnetospheres around the extreme Kerr black hole. In this case there is no known exact analytic solution to force free electrodynamics which is stationary, axisymmetric and magnetically-dominated. However, any stationary, axisymmetric and regular force-free magnetosphere in extreme Kerr black hole approaches the same attractor solution in the near-horizon extreme Kerr (NHEK) limit with null electromagnetic field. We show that by moving away from the attractor solution in the NHEK region, one finds magnetically-dominated solutions in the extreme Kerr black hole with finite angular momentum outflow. This result is achieved using a perturbative analysis up to the second order.
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